Skylab Refereed Journals


  1. Observation and implications of sub-iron and iron abundance ratios in low energy galactic cosmic rays.
    Durgaprasad, N et al., AdSpR, 15, 0149 (1995)
  2. Observations of sub-iron (Sc-Cr) to iron (Fe) abundance ratios in the low energy (30 - 300 MeV/N) galactic cosmic rays in Spacelab-3 experiment and their implications.
    Biswas, S et al., BASI, 21, 387 (1993)
  3. Neutron fluxes on board an orbital station
    Ryabeva, R et al., KosIs, 31, 118 (1993)
  4. SI II emission line diagnostics.
    Judge, P, Carpenter, K & Harper, G, MNRAS, 253, 123 (1991)
  5. Cosmic-ray neutron albedo dose in low-earth orbits
    Wilson, J, Townsend, L & Farhat, H, HeaPh, 57, 665 (1989)
  6. Integrated UV magnitudes of the Large Magellanic Cloud associations.
    Vuillemin, A, A&AS, 72, 249 (1988)
  7. Sub-iron to iron nuclei in low-energy (50 200 MeV nucl-1) cosmic rays as observed in the Skylab experiment
    Durgaprasad, N & Biswas, S, Ap&SS, 149, 163 (1988)
  8. Monte Carlo Particle Trajectory Models for Neutral Cometary Gases. I. Models and Equations
    Combi, M & Smyth, W, ApJ, 327, 1026 (1988)
  9. Atomic nuclei in the composition of the inner radiation belt of the earth.
    Nymmik, P, Ge&Ae, 25, 29 (1985)
  10. The Universe in X-rays.
    Henbest, N, NewSc, 93, 720 (1982)
  11. A classification system for O - B2 stars based on the Si IV and C IV resonance lines.
    Henize, K, Wray, J & Parsons, S, AJ, 86, 1658 (1981)
  12. Ultra-heavy cosmic ray studies with Ariel VI
    Fowler, P et al., Natur, 291, 45 (1981)
  13. Energy Source of the Solar Wind
    Carlqvist, P & Alfven, H, Ap&SS, 71, 203 (1980)
  14. SKYLAB Measurements of Low Energy Cosmic Rays
    Biswas, S & Durgaprasad, N, SSRv, 25, 285 (1980)
  15. HD 149499B : the hottest white dwarf ?
    Wray, J, Parsons, S & Henize, K, ApJL, 234, L187 (1979)
  16. Possible detection of energetic Jovian heavy ions at Skylab orbit
    Price, P, GeoRL, 6, 711 (1979)
  17. Charge states of low energy cosmic rays in the SKYLAB experiment
    Durgaprasad, N et al., IJRSP, 8, 222 (1979)
  18. Spectral types for early-type stars observed by Skylab.
    Roman, N, AJ, 83, 172 (1978)
  19. Charge and energy spectra of cosmic rays with Z ⪆ 60: the Skylab experiment.
    Shirk, E & Price, P, ApJ, 220, 719 (1978)
  20. Ultraheavy cosmic rays: theoretical implications of recent observations.
    Blake, J et al., ApJ, 221, 694 (1978)
  21. Solar-polar coronal holes and the north-south cosmic ray gradient
    Agrawal, S, Lanzerotti, L & Venkatesan, D, GeoRL, 5, 589 (1978)
  22. Thin aluminum filters for use on Apollo Telescope Mount XUV spectrograph.
    Schumacher, R & Hunter, W, ApOpt, 16, 904 (1977)
  23. Properties of low energy ions observed in the Skylab cosmic ray experiment.
    Biswas, S et al., IJRSP, 6, 209 (1977)
  24. Two UV colours of the central part of M31.
    Deharveng, J et al., A&A, 50, 371 (1976)
  25. Skylab ultraviolet stellar spectra: cool stars with hot secondaries.
    Parsons, S et al., ApJ, 203, 435 (1976)
  26. Skylab ultraviolet stellar spectra: a new white dwarf, HD 149499 B.
    Parsons, S et al., ApJL, 206, L71 (1976)
  27. Skylab ultraviolet stellar spectra: emission lines from the Beta Lyrae system.
    Kondo, Y et al., ApJ, 208, 468 (1976)
  28. A search for stellar soft X-ray sources.
    Vanderhill, M et al., ApJL, 197, L19 (1975)
  29. Skylab ultraviolet stellar spectra: variation of intensity and structure of strong lines with temperature and luminosity.
    Henize, K et al., ApJL, 199, L119 (1975)
  30. Skylab ultraviolet stellar spectra: the Wolf-Rayet stars.
    Henize, K et al., ApJL, 199, L173 (1975)
  31. Low energy cosmic ray ions observed in the Skylab experiment.
    Biswas, S et al., IJRSP, 4, 210 (1975)
  32. Enhanced abundances of Ca, Ti and Cr in low energy cosmic rays in Skylab experiment
    Biswas, S et al., Natur, 258, 409 (1975)
  33. Elemental abundances in interplanetary dust
    Brownlee, D et al., Natur, 252, 667 (1974)
  34. A Search for Soft Stellar X-Ray Sources.
    Vanderhill, M, PhD Thesis, 1 (1974)

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